Relativistic Hartree-Bogoliubov Calculation of Specific Heat of the Inner Crust of Neutron Stars

Details Relativistic Hartree-Bogoliubov Calculation of Specific Heat of the Inner Crust of Neutron Stars Relativistic Hartree-Bogoliubov Calculation of Specific Heat of the Inner Crust of Neutron Stars

2001-03-21

arxiv.org/abs/nucl-th/0103054v1

Prog.Theor.Phys. 112 (2004) 619-627

Physics

Nuclear Physics

Nuclear Theory

5 pages, Talk presented at the 3rd JAERI Symposium on Science of Hadrons under Extreme Conditions, January 2001

Scientific paper

10.1143/PTP.112.619

We calculate the specific heat of the inner crust of neutron stars within a local-density approximation to an improved relativistic Hartree-Bogoliubov theory. Non-uniformness of the system enhances the specific heat in particular at low temperatures. The degree of enhancement is similar to that in the spherical phase of Elgar{\o}y et al. We examine a schematic interpolation between the results of Broglia et al. adopting the Gogny force and ours based on the Lagrangian of the relativistic mean field model.

Affiliated with

Also associated with

No associations

Rating

Relativistic Hartree-Bogoliubov Calculation of Specific Heat of the Inner Crust of Neutron Stars does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Relativistic Hartree-Bogoliubov Calculation of Specific Heat of the Inner Crust of Neutron Stars, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Relativistic Hartree-Bogoliubov Calculation of Specific Heat of the Inner Crust of Neutron Stars will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-239486